Detector and readout characterization for POLARBEAR-2b
Detector and readout characterization for POLARBEAR-2b
复制标题
POLARBEAR-2b 的探测器和读数表征
DOI:
10.1117/12.2562766
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发表时间:
2020
期刊:
影响因子:
--
通讯作者:
Ito Jennifer et al.
中科院分区:
文献类型:
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作者:
大矢淳史;家城佳;大谷航;越智敦彦;Liang Haozhao;中野昇;Takahiro Nishinaka;干潟 紘太郎,森島 邦博,北川 暢子,西尾 晃,久野 光慧,眞部 祐太;Junya SUZUKI;Ito Jennifer et al.
The Simons Array is a set of three millimeter-wavelength telescopes in the Atacama Desert in northern Chile. It is designed to measure the polarization of the cosmic microwave background caused by density perturbations, gravitational lensing, and primordial gravitational waves. Polarbear-2b (PB-2b) is the receiver that will be mounted onto the Paul Simons Telescope, the second Simons Array telescope. Each pixel in the PB-2b focal plane has a broadband sinuous antenna coupled to transition-edge sensor (TES) bolometers. In all, there are more than 7,500 antenna-coupled TES bolometers which are biased and read out using a digital frequency-domain multiplexing framework. We implement a multiplexing factor of 40 with resonator frequencies ranging from 1.6 MHz to 4.6 MHz. These resonators are connected to superconducting quantum interference device arrays that provide a signal amplification stage. We present Polarbear-2b detector and readout characterization results from in-lab testing that enabled the deployment of PB-2b to Chile in March 2020.